Soft X-ray decline and cessation of pulsation in RS Oph

Details Soft X-ray decline and cessation of pulsation in RS Oph Soft X-ray decline and cessation of pulsation in RS Oph

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..801....1o&link_type=abstract

The Astronomer's Telegram, #801

Astronomy and Astrophysics

Astronomy

8

X-Ray, Novae

Scientific paper

The very bright super-soft X-ray phase of the recurrent nova RS Oph has been extensively observed by the Swift XRT. The highly variable soft X-ray flux reported in ATEL #764 and ATEL#770 stabilised significantly after 2006 Mar 31.4; the XRT observations have subsequently shown a linear decline between Apr 12.1 and Apr 28.7 from 208 to 98 c/s (0.2-10 keV, 100 c/s corresponds to 1.95e-8 erg/cm^2/s unabsorbed in this band).

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